Physics – Plasma Physics
Scientific paper
Dec 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufmsh33c..07o&link_type=abstract
American Geophysical Union, Fall Meeting 2010, abstract #SH33C-07
Physics
Plasma Physics
[2164] Interplanetary Physics / Solar Wind Plasma, [2169] Interplanetary Physics / Solar Wind Sources, [7859] Space Plasma Physics / Transport Processes, [7974] Space Weather / Solar Effects
Scientific paper
We study the temporal evolution and the spatial variation of the solar wind on different scales. The analyzed multi-spacecraft (STEREO, VEX, SOHO, MEX, and other spacecraft) measurements were obtained between 2007 and 2010 during solar minimum in the inner heliosphere. We derived the temporal and spatial variability of the different solar wind parameters (proton bulk velocity, electron core density, etc). These results support prediction of the solar wind parameters for different heliospheric positions and help to derive its validity range. In order to explain occasional deviations from the nominal solar wind evolution we use imaging data and modeling results.
Fedorov Arkady
Galvin Antoinette B.
Luhmann Janet G.
Opitz Andrea
Riley Pete
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